Newton's Second Law of Motion: F = ma

Newton's Second Law of Motion: F = ma

Assessment

Interactive Video

Physics, Science

11th Grade - University

Hard

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Quizizz Content

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The video tutorial covers Newton's first and second laws of motion, focusing on the equation F = ma. It explains how force, mass, and acceleration are related and discusses the concept of net force and vector addition. The tutorial also highlights the wide range of applications of Newton's second law, including calculating the masses of celestial objects.

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5 questions

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1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What does Newton's first law of motion state about an object's motion?

An object will accelerate unless acted upon by a net force.

An object will continue its state of motion unless acted upon by a net force.

An object will remain at rest unless acted upon by a net force.

An object will decelerate unless acted upon by a net force.

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

According to Newton's second law, what is the relationship between force, mass, and acceleration?

Force is equal to mass plus acceleration.

Force is equal to mass times acceleration.

Force is equal to acceleration divided by mass.

Force is equal to mass divided by acceleration.

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does the mass of an object affect the force required to achieve a certain acceleration?

Mass does not affect the force required.

Heavier objects require more force.

Heavier objects require less force.

Heavier objects require the same force as lighter objects.

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the net force acting on an object?

The average of all forces acting on the object.

The difference between the largest and smallest forces.

The largest force acting on the object.

The sum of all forces acting on the object.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How can Newton's second law be applied in astronomy?

To calculate the speed of light.

To determine the distance between stars.

To calculate the masses of celestial objects.

To measure the temperature of planets.